Hubble image archive

Compass and Scale Image of Cluster Galaxies

CreditsImage: NASA, ESA, and Z. Levay (STScI); Science: NASA, ESA, M. Donahue (Michigan State University), Y. Li (University of Michigan), G. Tremblay (Yale University), and R. Mittal (Rochester Insitute of Technology, and Max Planck Institute for Gravitational Physics)

Date
Jan 1, 2015
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2015-26-3608-image
By

Credits

Image: NASA, ESA, and Z. Levay (STScI);
Science: NASA, ESA, M. Donahue (Michigan State University), Y. Li (University of Michigan), G. Tremblay (Yale University), and R. Mittal (Rochester Insitute of Technology, and Max Planck Institute for Gravitational Physics)

Image Details

About The Object
Object NameMACS J1931, MACS J1532, Abell 1664, Abell 1795, Abell 2597, Hydra A, RX J1504, ZwCl 8193
Object DescriptionBrightest Cluster Galaxies (BCG)
About The Data
Data DescriptionData for galaxies taken with the WFC3/UVIS instrument were obtained as part of the CLASH proposal: , PI: M. Postman (STScI) et al. Data for galaxies taken with the ACS/SBC instrument were obtained from proposal: , PI: R. Mittal (Max Planck Institute for Gravitational Physics) et al. The WFC3/UVIS BCG science team comprises: M. Donahue and T. Connor (Michigan State University), K. Fogarty (STScI), Y. Li (University of Michigan, Ann Arbor), M. Voit (Michigan State University), M. Postman and A. Koekemoer (STScI), J. Moustakas (Siena College, NY), L. Bradley (STScI), and H. Ford (JHU). The ACS/SBC BCG science team comprises: G. Tremblay (Yale University/ESO), C. O’Dea and S. Baum (University of Manitoba/RIT), R. Mittal (RIT/Max Planck Institute for Gravitational Physics), M. McDonald (Kavli Institute/MIT), F. Combes (Observatoire de Paris/CNRS), Y. Li (University of Michigan, Ann Arbor), B. McNamara (Waterloo University, Ontario/Harvard-Smithsonian Center for Astrophysics), M. Bremer (University of Bristol, UK), T. Clarke (Naval Research Laboratory), M. Donahue (Michigan State University), A. Edge (Durham University), A. Fabian (Institute of Astronomy), S. Hamer (Observatoire de Paris/CNRS), M. Hogan (Waterloo University, Ontario), J. Oonk (Netherlands Institute for Radio Astronomy), A. Quillen (University of Rochester), J. Sanders (Max Planck Institute for Extraterrestrial Physics), P. Salomé (Observatoire de Paris/CNRS), and M. Voit (Michigan State University).
InstrumentHST>WFC3/UVIS and HST>ACS/SBC

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